3D WKB solution for fast magnetoacoustic wave behaviour within a separatrix dome containing a coronal null point

James A. McLaughlin (Lead / Corresponding author), Jonathan O. Thurgood, Gert J. J. Botha, Joshua A. Wiggs

Research output: Contribution to journalArticle

Abstract

The propagation of the fast magnetoacoustic wave is studied within a magnetic topology containing a 3D coronal null point whose fan field lines form a dome. The topology is constructed from a magnetic dipole embedded within a global uniform field. This study aims to improve the understanding of how magnetohydrodynamics (MHD) waves propagate through inhomogeneous media, specifically in a medium containing an isolated 3D magnetic null point. We consider the linearized MHD equations for an inhomogeneous, ideal, cold plasma. The equations are solved utilizing the WKB approximation and Charpit’s Method. We find that for a planar fast wave generated below the null point, the resultant propagation is strongly dependent upon initial location and that there are two main behaviours: the majority of the wave escapes the null (experiencing different severities of refraction depending upon the interplay with the equilibrium Alfvén-speed profile) or, alternatively, part of the wave is captured by the coronal null point (for elements generated within a specific critical radius about the spine and on the z = 0 plane). We also generalize the magnetic topology and find that the height of the null determines the amount of wave that is captured. We conclude that for a wavefront generated below the null point, nulls at a greater height can trap proportionally less of the corresponding wave energy.

Original languageEnglish
Pages (from-to)1390-1400
Number of pages11
JournalMonthly Notices of the Royal Astronomical Society
Volume484
Issue number1
Early online date16 Jan 2019
DOIs
Publication statusPublished - Mar 2019

Fingerprint

magnetoacoustic waves
domes
dome
topology
magnetohydrodynamics
Wentzel-Kramer-Brillouin method
spine
propagation
cold plasmas
magnetohydrodynamic waves
fans
magnetic dipoles
escape
refraction
wave energy
traps
radii
plasma
profiles
approximation

Keywords

  • (magnetohydrodynamics) MHD
  • Magnetic fields
  • Sun: corona
  • Waves

Cite this

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abstract = "The propagation of the fast magnetoacoustic wave is studied within a magnetic topology containing a 3D coronal null point whose fan field lines form a dome. The topology is constructed from a magnetic dipole embedded within a global uniform field. This study aims to improve the understanding of how magnetohydrodynamics (MHD) waves propagate through inhomogeneous media, specifically in a medium containing an isolated 3D magnetic null point. We consider the linearized MHD equations for an inhomogeneous, ideal, cold plasma. The equations are solved utilizing the WKB approximation and Charpit’s Method. We find that for a planar fast wave generated below the null point, the resultant propagation is strongly dependent upon initial location and that there are two main behaviours: the majority of the wave escapes the null (experiencing different severities of refraction depending upon the interplay with the equilibrium Alfv{\'e}n-speed profile) or, alternatively, part of the wave is captured by the coronal null point (for elements generated within a specific critical radius about the spine and on the z = 0 plane). We also generalize the magnetic topology and find that the height of the null determines the amount of wave that is captured. We conclude that for a wavefront generated below the null point, nulls at a greater height can trap proportionally less of the corresponding wave energy.",
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3D WKB solution for fast magnetoacoustic wave behaviour within a separatrix dome containing a coronal null point. / McLaughlin, James A. (Lead / Corresponding author); Thurgood, Jonathan O.; Botha, Gert J. J.; Wiggs, Joshua A.

In: Monthly Notices of the Royal Astronomical Society, Vol. 484, No. 1, 03.2019, p. 1390-1400.

Research output: Contribution to journalArticle

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